Our star can light worlds—and shut them down. This episode traces the Sun’s hidden machinery from the first recorded superstorm to the moment a probe “touched” its atmosphere.

Discover how Galileo’s sunspots became Schwabe’s 11-year cycle, why Birkeland’s aurora theory was dismissed then proven, and how Ulysses, SOHO, and SDO changed what we thought was knowable. See the SOHO near-loss and recovery that rewrote its software, the MMS mission catching magnetic reconnection in action, and the Van Allen probes spotting a surprise third radiation belt that vanished in days. Then ride along as Parker Solar Probe slips inside the Alfvén boundary and follows violent magnetic switchbacks back to their source—while Solar Orbiter delivers the closest images yet. Finally, witness the stakes on Earth: Quebec’s 1989 grid failure, Starlink’s 38-satellite loss after a mistimed launch, and why “space weather” forecasts now matter to everyone with power, GPS, or internet.

Watch to connect the breakthroughs—and the risks—and see how new missions (including Prober-3) aim to predict the Sun’s next move.

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